G180-24
taken from 8 paper(s):
/J.Simmerer et al.(2004)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/I.U.Roederer et al.(2010)/
/H.L.Yan et al.(2016)/
/A.M.Boesgaard et al.(2011)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 6059 | log g : 4.09 | vturb : 0.50 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | -0.5 | ... | -1.66 | -0.32 | 6.77 | C |
Fe I | 6 | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe I |
Fe II | 8 | -1.30 | ... | ... | -1.30 | ... | 6.20 | Fe II |
La II | N/A | ... | ... | -0.19+-0.11 | -1.29+-0.11 | 0.05+-0.11 | -0.19+-0.11 | La II |
Eu II | N/A | ... | ... | -0.58+-0.06 | -1.10+-0.06 | 0.24+-0.06 | -0.58+-0.06 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 6108+-111 | log g : 4.12+-0.31 | vturb : 1.43+-0.09 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | N/A | ... | ... | 2.35+-0.08 | -0.91+-0.08 | 0.45+-0.08 | 2.35+-0.08 | Li I |
Fe | N/A | -1.38+-0.06 | ... | ... | -1.36+-0.06 | ... | 6.14+-0.06 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 240 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 6108+-111 | log g : 4.12+-0.31 | vturb : 1.43+-0.09 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | N/A | -1.48+-0.08 | -0.08+-0.09 | ... | -1.39+-0.08 | 0.00+-0.09 | 4.85+-0.08 | Na I |
Mg I | N/A | -1.04+-0.05 | +0.36+-0.08 | ... | -1.06+-0.05 | 0.33+-0.08 | 6.54+-0.05 | Mg I |
Si | N/A | ... | +0.24+-0.12 | ... | -1.12+-0.12 | 0.27+-0.12 | 6.39+-0.12 | Si |
Si I | 3 | -1.03+-0.15 | ... | ... | -0.99+-0.15 | 0.40+-0.15 | 6.52+-0.15 | Si I |
Si II | 1 | -1.30+-0.16 | ... | ... | -1.26+-0.16 | 0.13+-0.16 | 6.25+-0.16 | Si II |
Ca I | N/A | -1.07+-0.08 | +0.33+-0.10 | ... | -1.05+-0.08 | 0.34+-0.10 | 5.29+-0.08 | Ca I |
Ti | N/A | ... | +0.31+-0.07 | ... | -1.05+-0.07 | 0.34+-0.07 | 3.90+-0.07 | Ti |
Ti I | 13 | -1.10+-0.06 | ... | ... | -1.06+-0.06 | 0.33+-0.06 | 3.89+-0.06 | Ti I |
Ti II | 7 | -1.06+-0.08 | ... | ... | -1.02+-0.08 | 0.37+-0.08 | 3.93+-0.08 | Ti II |
Cr | N/A | ... | -0.04+-0.08 | ... | -1.41+-0.08 | -0.02+-0.08 | 4.23+-0.08 | Cr |
Cr I | 13 | -1.45+-0.06 | ... | ... | -1.42+-0.06 | -0.03+-0.06 | 4.22+-0.06 | Cr I |
Cr II | 4 | -1.34+-0.21 | ... | ... | -1.31+-0.21 | 0.08+-0.21 | 4.33+-0.21 | Cr II |
Fe | N/A | -1.40+-0.05 | ... | ... | -1.39+-0.05 | ... | 6.11+-0.05 | Fe |
Fe I | 56 | -1.38+-0.07 | ... | ... | -1.37+-0.07 | ... | 6.13+-0.07 | Fe I |
Fe II | 11 | -1.44+-0.09 | ... | ... | -1.43+-0.09 | ... | 6.07+-0.09 | Fe II |
Ni I | N/A | -1.46+-0.10 | -0.06+-0.12 | ... | -1.43+-0.10 | -0.04+-0.12 | 4.79+-0.10 | Ni I |
Y II | N/A | -1.23+-0.10 | +0.17+-0.12 | ... | -1.20+-0.10 | 0.19+-0.12 | 1.01+-0.10 | Y II |
Ba II | N/A | -1.08+-0.46 | +0.32+-0.46 | ... | -1.13+-0.46 | 0.26+-0.46 | 1.05+-0.46 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2450889.494 | MAYALLKPNO | 35000 | 240 | 1200 | -150.8+-0.6 |
THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Zn I | N/A | ... | ... | 3.23 | -1.33 | 0.01 | 3.23 | Zn I |
Y II | N/A | ... | ... | 0.72 | -1.49 | -0.15 | 0.72 | Y II |
Pb I | N/A | ... | ... | <+1.65 | <-0.39 | <0.95 | <+1.65 | Pb I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 6004 | log g : 4.21 | vturb : 1.5 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -1.39 | ... | ... | -1.39 | ... | 6.11 | Fe |
Cu | N/A | ... | -0.46+-0.00 | ... | -1.83+-0.00 | -0.44+-0.00 | 2.36+-0.00 | Cu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FIESNOT | 40000 | 140-200 | N/A | N/A |
Beryllium and Alpha-element Abundances in a Large Sample of Metal-poor Stars
Stellar Parameters
Teff : 6008+-100 | log g : 3.77+-0.2 | vturb : 1.31+-0.2 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Be | N/A | ... | -0.16+-0.15 | -0.18+-0.12 | -1.56+-0.12 | -0.12+-0.15 | -0.18+-0.12 | Be |
O | N/A | -0.88+-0.22 | +0.56+-0.24 | ... | -0.94+-0.22 | 0.50+-0.24 | 7.75+-0.22 | O |
Mg | N/A | -1.06+-0.07 | ... | ... | -1.08+-0.07 | 0.36+-0.07 | 6.52+-0.07 | Mg |
Ti | N/A | -1.16+-0.09 | ... | ... | -1.09+-0.09 | 0.35+-0.09 | 3.86+-0.09 | Ti |
Fe | N/A | -1.44+-0.09 | ... | ... | -1.44+-0.09 | ... | 6.06+-0.09 | Fe |
Position
Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-19 | N/A | KECKHIRES | 42000 | 86 | 1800 | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 6004 | log g : 4.21 | vturb : 1.5 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na | N/A | ... | -0.14 | ... | -1.44 | -0.05 | 4.80 | Na |
Mg | N/A | ... | 0.31 | ... | -1.10 | 0.29 | 6.50 | Mg |
Si | N/A | ... | 0.31 | ... | -1.04 | 0.35 | 6.47 | Si |
Ca | N/A | ... | 0.39 | ... | -0.98 | 0.41 | 5.36 | Ca |
Ti | N/A | ... | 0.31 | ... | -1.01 | 0.38 | 3.94 | Ti |
Cr | N/A | ... | 0.03 | ... | -1.33 | 0.06 | 4.31 | Cr |
Fe | N/A | -1.39 | ... | ... | -1.39 | ... | 6.11 | Fe |
Ni | N/A | ... | -0.04 | ... | -1.40 | -0.01 | 4.82 | Ni |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-18-0134 | N/A | FIESNOT | 40000 | 170 | N/A | -152 |
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Mn | N/A | ... | -0.34 | ... | -1.77 | -0.38 | 3.66 | Mn |
Fe | N/A | -1.39 | ... | ... | -1.39 | ... | 6.11 | Fe |
Cu | N/A | ... | -0.43 | ... | -1.80 | -0.41 | 2.39 | Cu |
Zn | N/A | ... | 0.12 | ... | -1.23 | 0.16 | 3.33 | Zn |
Y | N/A | ... | 0.07 | ... | -1.29 | 0.10 | 0.92 | Y |
Ba | N/A | ... | -0.18 | ... | -1.62 | -0.23 | 0.56 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-18-0134 | N/A | FIESNOT | 40000 | 170 | N/A | -152 |